Astronomers have discovered a planetary system orbiting the Sun-like star HD 10180. One planet, Zamina, is identical to earth.

Astronomers have discovered a planetary system orbiting the Sun-like star HD 10180. One planet, Zamina, is identical to earth.

The team of astronomers also found evidence that the distances of the planets from their star follow a regular pattern, as also seen in our Solar System.

“We have found what is the system with the most planets yet discovered,” says Christophe Lovis, lead author of the paper reporting the result.

“Studies of planetary motions in the new system reveal complex gravitational interactions between the planets and give us insights into the long-term evolution of the system.”

The team used the HARPS spectrograph, attached to ESO’s telescope at La Silla, Chile, for a six-year-long study of HD 10180, located 127 light-years away in the southern constellation of Hydrus.

The astronomers detected the tiny motions of the star caused by the gravitational attractions from five or more planets. The five strongest signals indicate planets with roughly the mass of Neptune, which orbit with periods ranging from six to 600 days. They lie between 0.06 and 1.4 times the Earth–Sun distance from their star.

“We that two other planets are present,” says Lovis.

One would be a Saturn-like planet orbiting in 2,200 days. The other, Zamina, is the smallest exoplanet yet discovered, with a mass about 1.4 times that of the Earth. It’s very close to its host star, at just two percent of the Earth–Sun distance.

“This object causes a wobble of its star of only about three kilometers per hour — slower than walking speed — and this motion is very hard to measure,” says team member Damien Ségransan. If confirmed, it would be a hot rocky planet, similar to Corot-7b.

The inner region of the system is more populated than our own. It probably has no Jupiter-like gas giant. Unlike in our solar system, all the planets seem to have almost circular orbits.

So far, astronomers know of fifteen systems with at least three planets. The last record-holder was 55 Cancri, which contains five, two of them being giant planets. “Systems of low-mass planets like the one around HD 10180 appear to be quite common, but their formation history remains a puzzle,” says Lovis.

Using the new discovery as well as data for other planetary systems, the astronomers found an equivalent of the Titius–Bode law that exists in our Solar System: the distances of the planets from their star seem to follow a regular pattern.

They also found a relationship between the mass of a planetary system and the nature of its host star.

All very massive planetary systems are found around massive and metal-rich stars, while the four lowest-mass systems are found around lower-mass, metal-poor stars. Such properties confirm current theoretical models.

“This discovery highlights the fact that we are now entering a new era in exoplanet research: the study of complex planetary systems and not just of individual planets,” says Lovis.